Hence, the smaller
the value of \(\epsilon \) , the greater would be the order-of-magnitude enhancement of \(m\) , which is
in fact desirable from the point of view of preventing small-scale structure formation of
the CDM because of the uncertainty principle
[1]}.
Such a relative mass enhancement with decreasing \(\epsilon \)  (from its limiting value of about \(0.1\) 
found above) is shown in Fig. REF , alongwith the \(\epsilon \) -variation of the BEC density
parameter at the present epoch, \(\Omega ^{\mbox{\tiny ({\it B})}}_{_0}\equiv [\rho ^{(B)}/\rho ]\big \vert _{t = t_{_0}}\) , obtained from
Eq. (REF ). In all the
requisite calculations for these plots, we have used the best fit values of the
Planck 2018 TT,TE,EE+lowE+Lensing+BAO parametric estimations for \(\Lambda \) CDM quoted in the
Eq. (REF ) above.
